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08 February 2022 | Story Anthony Mthembu | Photo Charl Devenish
Dr Munita Dunn-Coetzee
“I would like for students to walk in here and feel comfortable; it doesn’t matter what you identify as – there is a space for you here,” says Dr Munita Dunn-Coetzee, the new Director of Student Counselling and Development.

Dr Munita Dunn-Coetzee has joined the University of the Free State as the new Director of Student Counselling and Development. This is after an eleven-year stay at Stellenbosch University as the Deputy Director of the Centre for Student Structures and Communities, and later as the Director of the Centre for Student Counselling and Development.

Dr Dunn-Coetzee’s role at the UFS

As leader of the department, Dr Dunn-Coetzee sees her role as one in which she is responsible for moving her team forward. “My role is to really look at what the team needs. This is from infrastructure right through to their own personal development, and to making sure that they have what they need to get their jobs done,” she stated. In addition, Dr Dunn-Coetzee’s responsibilities include, “looking at our strategic intent, aligning with what the university wants, being relevant in terms of our service delivery, and connecting enough with the students”. In fact, one of the things she is excited about is learning from the students at the University of the Free State. “The big thing for me is to make contact with students and to engage with them about what is going on at ground level; the one thing I don’t want to be is someone who sits in the office, sends emails, and think I know what’s going on,” she explained.

A commitment to the mental health of UFS students

Although her two predecessors were internal appointments, Dr Dunn-Coetzee argues that being an external appointment allows her to have a fresh perspective. As such, one of her main priorities for the year is looking at student leaders, day residences, residences on campus, and residential heads, and analysing whether they are empowered enough to have conversations about mental-health issues with students. “The one thing that concerns me is that we have been online for two years, and now that we are telling students to come back to campus, it might evoke a level of anxiety in some students,” she explained. Therefore, ensuring that the department is student-centred in everything it does is very important to Dr Dunn-Coetzee. This varies from the way in which students are dealt with, how emails are responded to, and how students are treated when they walk into the Kovsie Health Building.

A long-term vision for the department and the university

Even though she has not been at the University of the Free State for very long, Dr Dunn-Coetzee has some long-term goals that are bound to positively impact both the students and the staff in her department. “I would like to have a research focus within our department; it is very easy to say that we are doing good work and that we have an impact on our students, but we need to have something that proves it,” she said. Therefore, an evidence-based approach is one of the directions she would like to pursue in her department. In addition, Dr Dunn-Coetzee argues that there is a need for a space in which intern psychologists can be trained. “It keeps your current staff on their toes, and it helps you to really play a role in developing psychologists in South Africa,” she expressed. Therefore, opening this space for young psychologists is something she hopes to make a reality in her time at the university. Furthermore, developing her staff and ensuring that they grow their skill set is an important goal she would like to achieve. “My focus is not to have people work here for thirty years; I need to empower them so that they can develop as much as they can. Of course, I love having them here, but in the event that they want to work somewhere else I need to make sure that they are skilled,” she said. Lastly, a goal she is adamant to achieve is to ensure that the service delivery by Student Counselling and Development is of a high standard on all three campuses.

As such, Dr Dunn-Coetzee would like to be viewed by the student community as accessible and approachable. “I would like for students to walk in here and feel comfortable; it doesn’t matter what you identify as – there is a space for you here,” she said.

News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

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